Slide 1
How do they work?
Slide 2
1. History
2. Lenses & Hardware
3. Reflecting Telescopes
4. Refracting Telescopes
Slide 3
Hans Lippershey Middleburg, Holland
invented the refractor telescope in 1608
Galileo
the first to use a telescope in astronomy. Galileo's designs used a combination of convex and concave lenses.
Kepler
improved the design to have two convex lenses, which made the image upside-down. Kepler's design is still the major design of refractors today, with a few later improvements in the lenses and the glass to make them.
Slide 4
The answer is simple: the object does not take up much space on your eye’s screen (retina).
Using a digital camera analogy, at 150 feet the writing on a dime does not cover enough pixels on your retinal sensor for you to read the writing.
This can be corrected by bending the light with lenses.
Slide 5
The lens in your eyes works like a glass lens. The light bends as it goes through a different medium.
Light rays are bent when they intersect glass; a curved surface can produce an image.
In your eye, the image is then focused at the retina.
Slide 6
If you had a bigger eye, you could collect more light from the object. This image could be magnified so it stretches out over more pixels in your retina.
In a telescope, two pieces make this possible:
the objective lens (refractor telescopes) or primary mirror (reflecting telescopes)
the eye piece
Slide 7
The objective lens (in refractors) or primary mirror (in reflectors) collects lots of light from a distant object and brings that light, or image, to a point or focus.
An eyepiece lens takes the bright light from the focus of the objective lens or primary mirror and "spreads it out" (magnifies it) to take up a large portion of the retina. This is the same principle that a magnifying glass (lens) uses; it takes a small image on the paper and spreads it out over the retina of your eye so that it looks big.
Slide 8
Slide 9